he SYK TENSOR Quantum Information Network (QIN): Resolution of the Cosmological Constant Problem and Dark Energy via Finite-Capacity Chaotic Qubit Substrate, Scrambling Backreaction, and Soft Regulated UV Finiteness (Empirically Validated with Large Scale Statistics and Exact 1/N² Derivation)

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Authors: Stanley Preschutti
Cited by: 0

Abstract

The cosmological constant problem why the observed dark energy density is Λobserved ≈10−120 in Planck units rather than ∼ O(1) is resolved naturally and completely within theSYK TENSOR Quantum Information Network (QIN). Reality emerges from a discrete, finitecapacity substrate of maximally chaotic Majorana qubits governed by random all-to-all SYKinteractions, stabilized by holographic tensor network error correction, and softly regulated withGaussian form factors (stability coefficient γ ≈ 1.0–1.2). Naive vacuum energy contributions areexponentially suppressed by finite global qubit number N, yielding ρvac ∼ exp(−cN) ≪ 10−120.A tiny positive residual cosmological constant Λ ≈ λ2L/N2 emerges directly from finite-sizecorrections to OTOC scrambling saturation. Setting N ≈ 10120–10122 reproduces Λobservedexactly without fine tuning

Fields of Study & Subjects

Cosmology and Gravitation Theories Noncommutative and Quantum Gravity Theories Black Holes and Theoretical Physics

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
9 February 2026
Language
EN